5. Work, energy and power
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5.1 Energy conservation
• understand the concept of work, and recall and use work done = force × displacement in the direction of the force
• recall and apply the principle of conservation of energy
• recall and understand that the efficiency of a system is the ratio of useful energy output from the system to the total energy input
• use the concept of efficiency to solve problems
• define power as work done per unit time
• solve problems using P = W / t
• derive P = Fv and use it to solve problems
5.2 Gravitational potential energy and kinetic energy
5.2.1W = Fs, the formula ∆EP = mg∆h for gravitational potential energy changes in
• derive, using W = Fs, the formula ∆EP = mg∆h for gravitational potential energy changes in a uniform gravitational field
5.2.2The formula ∆EP = mg∆h for gravitational potential energy changes in a
• recall and use the formula ∆EP = mg∆h for gravitational potential energy changes in a uniform gravitational field
5.2.3The equations of motion, the formula for kinetic energy EK = 1/2 mv2
• derive, using the equations of motion, the formula for kinetic energy EK = 1/2 mv2
5.2.4EK = 1/2 mv2
• recall and use EK = 1/2 mv2